Using planetary nebulae to probe the structure of the galactic thin disk
Most planetary nebulae appear to arise from progenitors with mass MPG 1 M. One would therefore expect them to be closely associated with stars locatedwithin the galactic thin disk. This has been confrmed through a series of recentestimates of scale height, which imply values z0(PNe) of order 220 pc...
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| I publikationen: | Revista Mexicana de Astronomía y Astrofísica |
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| Huvudupphov: | |
| Materialtyp: | Artigo |
| Språk: | Inglês |
| Utgiven: |
Universidad Nacional Autónoma de México
2005
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| Ämnen: | |
| Länkar: | https://www.redalyc.org/articulo.oa?id=57141205 |
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